Forecast for cosmological parameter estimation with gravitational-wave standard siren observation from the Cosmic Explorer

Abstract

The third-generation ground-based gravitational-wave (GW) detector, Cosmic Explorer (CE), is scheduled to start its observation in the 2030s. In this paper, we make a forecast for cosmological parameter estimation with gravitational-wave standard siren observation from the CE. We use the simulated GW standard siren data of CE to constrain the $\Lambda$CDM, $w$CDM and CPL models. We combine the simulated GW data with the current cosmological electromagnetic observations including the latest cosmic microwave background anisotropies data from Planck, the optical baryon acoustic oscillation measurements, and the type Ia supernovae observation (Pantheon compilation) to do the analysis. We find that the future standard siren observation from CE will improve the cosmological parameter estimation to a great extent, since the future GW standard siren data can well break the degeneracies generated by the optical observations between various cosmological parameters. We also find that the CE's constraining capability on the cosmological parameters is slightly better than that of the same-type GW detector, the Einstein Telescope. In addition, the synergy between the GW standard siren observation from CE and the 21 cm emission observation from SKA is also discussed.

arXiv comment17 pages, 4 figures

References in corpus (39)

• Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
• Measurements of Omega and Lambda from 42 High-Redshift Supernovae
• GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
• Multi-messenger Observations of a Binary Neutron Star Merger
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
• The Complete Light-curve Sample of Spectroscopically Confirmed Type Ia Supernovae from Pan-STARRS1 and Cosmological Constraints from The Combined Pantheon Sample
• The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant
• TianQin: a space-borne gravitational wave detector
• The Clustering of the SDSS DR7 Main Galaxy Sample I: A 4 per cent Distance Measure at z=0.15
• Exploring the Sensitivity of Next Generation Gravitational Wave Detectors
• A gravitational-wave standard siren measurement of the Hubble constant
• Physics, Astrophysics and Cosmology with Gravitational Waves
• The missing link: Merging neutron stars naturally produce jet-like structures and can power short Gamma-Ray Bursts
• Cosmology with Phase 1 of the Square Kilometre Array; Red Book 2018: Technical specifications and performance forecasts
• Ultra-high precision cosmology from gravitational waves
• Determination of Dark Energy by the Einstein Telescope: Comparing with CMB, BAO and SNIa Observations
• Cosmography with the Einstein Telescope
• Science with the space-based interferometer eLISA. III: Probing the expansion of the Universe using gravitational wave standard sirens
• Distance Priors from Planck Final Release
• Estimating cosmological parameters by the simulated data of gravitational waves from the Einstein Telescope
• Gravitational waves from cosmological compact binaries
• The Local Rate and the Progenitor Lifetimes of Short-Hard Gamma-Ray Bursts: Synthesis and Predictions for LIGO
• Precision cosmology from future lensed gravitational wave and electromagnetic signals
• Science with the TianQin observatory: Preliminary results on massive black hole binaries
• Fundamentals of the orbit and response for TianQin
• Localization accuracy of compact binary coalescences detected by the third-generation gravitational-wave detectors and implication for cosmology
• Forecasts on the Dark Energy and Primordial Non-Gaussianity Observations with the Tianlai Cylinder Array
• Impacts of gravitational-wave standard siren observation of the Einstein Telescope on weighing neutrinos in cosmology
• Science with the TianQin observatory: Preliminary results on testing the no-hair theorem with ringdown signals
• Comparison of dark energy models after Planck 2015
• Constraining the time variation of Newton's constant $G$ with gravitational-wave standard sirens and supernovae
• Gravitational wave standard sirens and cosmological parameter measurement
• Cosmological parameter estimation with future gravitational wave standard siren observation from the Einstein Telescope
• Improving cosmological parameter estimation with the future gravitational-wave standard siren observation from the Einstein Telescope
• Precise measurements of inflationary features with 21 cm observations
• Prospect for constraining holographic dark energy with gravitational wave standard sirens from the Einstein Telescope
• Hyperunified field theory and Taiji program in space for GWD
• Improving cosmological parameter estimation with the future 21 cm observation from SKA
• Model-independent measurement of the absolute magnitude of Type Ia Supernovae with gravitational-wave sources

Cited by in corpus (57)

• Cosmology with the Laser Interferometer Space Antenna
• The Gravitational-Wave Physics II: Progress
• Forecast for cosmological parameter estimation with gravitational-wave standard sirens from the LISA-Taiji network
• A Program for Multi-Messenger Standard Siren Cosmology in the Era of LIGO A+, Rubin Observatory, and Beyond
• Prospects for improving cosmological parameter estimation with gravitational-wave standard sirens from Taiji
• Listening to the Universe with Next Generation Ground-Based Gravitational-Wave Detectors
• Cosmological parameter estimation for dynamical dark energy models with future fast radio burst observations
• Constraints on the distance duality relation with standard sirens
• The Taiji-TianQin-LISA network: Precisely measuring the Hubble constant using both bright and dark sirens
• Synergy between CSST galaxy survey and gravitational-wave observation: Inferring the Hubble constant from dark standard sirens
• A preliminary forecast for cosmological parameter estimation with gravitational-wave standard sirens from TianQin
• Cosmology with Standard Sirens at Cosmic Noon
• Measuring the Hubble constant with black sirens
• Prospects for measuring the Hubble constant and dark energy using gravitational-wave dark sirens with neutron star tidal deformation
• Impacts of gravitational-wave standard siren observations from Einstein Telescope and Cosmic Explorer on weighing neutrinos in interacting dark energy models
• Using a multi-messenger and multi-wavelength observational strategy to probe the nature of dark energy through direct measurements of cosmic expansion history
• A path to precision cosmology: synergy between four promising late-universe cosmological probes
• Quantifying the impacts of future gravitational-wave data on constraining interacting dark energy
• Prospects for probing the interaction between dark energy and dark matter using gravitational-wave dark sirens with neutron star tidal deformation
• On an alternative mechanism for the black hole echoes
• Cosmology with fast radio bursts in the era of SKA
• A new way to explore cosmological tensions using gravitational waves and strong gravitational lensing
• Dancing in the dark: detecting a population of distant primordial black holes
• Joint constraints on cosmological parameters using future multi-band gravitational wave standard siren observations
• Cosmology with the Einstein Telescope: No Slip Gravity Model and Redshift Specifications
• Prospects for constraining interacting dark energy models from gravitational wave and gamma ray burst joint observation
• A forecast of using fast radio burst observations to constrain holographic dark energy
• Exploring non-singular black holes in gravitational perturbations
• A comprehensive forecast for cosmological parameter estimation using joint observations of gravitational waves and short $\gamma$-ray bursts
• Prospects for measuring dark energy with 21 cm intensity mapping experiments: A joint survey strategy
• Cosmological model-independent measurement of cosmic curvature using distance sum rule with the help of gravitational waves
• Cosmography with Standard Sirens from the Einstein Telescope
• Efficient parameter inference for gravitational wave signals in the presence of transient noises using temporal and time-spectral fusion normalizing flow
• Null test for cosmic curvature using Gaussian process
• Searching for modified gravity in the astrophysical gravitational wave background: Application to ground-based interferometers
• Measuring the Hubble constant with coalescences of binary neutron star and neutron star-black hole: bright sirens \& dark sirens
• Model-independent $H_0$ within FLRW: Joint constraints from GWTC-3 standard sirens and strong lensing time delays
• Standard siren cosmology in the era of the 2.5-generation ground-based gravitational wave detectors: bright and dark sirens of LIGO Voyager and NEMO
• Eliminating polarization leakage effect for neutral hydrogen intensity mapping with deep learning
• Improving the Cosmological Constraints by Inferring the Formation Channel of Extreme-mass-ratio Inspirals
• HI intensity mapping with MeerKAT: forecast for delay power spectrum measurement using interferometer mode
• Prospects for weighing neutrinos in interacting dark energy models using joint observations of gravitational waves and $\gamma$-ray bursts
• Robust inference of gravitational wave source parameters in the presence of noise transients using normalizing flows
• Rapid identification of time-frequency domain gravitational wave signals from binary black holes using deep learning
• A Standard Siren Cosmological Measurement from the Potential GW190521 Electromagnetic Counterpart ZTF19abanrhr
• Fundamental Physics and Cosmology with TianQin
• Exploring the potentiality of standard sirens to probe cosmic opacity at high redshifts
• Revisiting holographic dark energy from the perspective of multi-messenger gravitational wave astronomy: future joint observations with short gamma-ray bursts
• Prospects for searching for sterile neutrinos with gravitational wave and $\gamma$-ray burst joint observations
• Prospects for cosmological research with the FAST array: 21-cm intensity mapping survey observation strategies
• Multi-messenger standard-siren cosmology for third-generation gravitational-wave detectors: forecasts considering observations of gamma-ray bursts and kilonovae
• Ultra-low-frequency gravitational waves from individual supermassive black hole binaries as standard sirens
• FAST Drift Scan Survey for HI Intensity Mapping. II. Stacking-based Beam Construction of the 19-feed Array at $1.4$ GHz
• Cosmological perturbations in the energy-momentum squared gravity theory: constraints from gravitational wave standard sirens and redshift space distortions
• Search for exotic gravitational wave signals beyond general relativity using deep learning
• Synergy between CSST and third-generation gravitational-wave detectors: Inferring cosmological parameters using cross-correlation of dark sirens and galaxies
• Prospects for joint multiband detection of intermediate-mass black holes by LGWA and the Einstein Telescope